{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:ZMIQ2UJ7COZZN24ZE6NP7OXV32","short_pith_number":"pith:ZMIQ2UJ7","schema_version":"1.0","canonical_sha256":"cb110d513f13b396eb99279affbaf5de975fb159356fc7bc3bec7c6cfd8c68c5","source":{"kind":"arxiv","id":"1912.03262","version":2},"attestation_state":"computed","paper":{"title":"CODEX clusters. The Survey, the Catalog, and Cosmology of the X-ray Luminosity Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Finoguenov, C. C. Kirkpatrick, E. Rozo, E. Rykoff, F. Kaefer, G. Erfanianfar, J. Comparat, J. Ider Chitham, J. Patrick Henry, J-P. Kneib, J. Weller, K. Kiiveri, L. van Waerbeke, M. Costanzi, N. Clerc, R. Capasso, R. Dupke, S. Damsted, S. Hagstotz, V. Lindholm","submitted_at":"2019-12-06T17:59:22Z","abstract_excerpt":"Large area catalogs of galaxy clusters constructed from ROSAT All Sky Survey provide the base for our knowledge on the population of clusters thanks to the long-term multiwavelength efforts on their follow-up. Advent of large area photometric surveys superseding in depth previous all-sky data allows us to revisit the construction of X-ray cluster catalogs, extending the study to lower cluster masses and to higher redshifts and to provide the modelling of the selection function. We perform a wavelet detection of X-ray sources and make extensive simulations of the detection of clusters in the RA"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1912.03262","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2019-12-06T17:59:22Z","cross_cats_sorted":[],"title_canon_sha256":"1ea962f10d115037c1710ababd6444be82ef8c1868fad5abe6234b977b66eae8","abstract_canon_sha256":"2a6c03345dbc045247a4cdd80ca97d7b265ef2938fbccb23d30a740c4b741fc7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:15:08.797068Z","signature_b64":"iX+w62Mns+xlXt6q358K7J6ouPnIbStXhP43zeCU8bopVkDs8WCZ/twusvl4LDaADmqHIeJy00KqAEn7XJ8fCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cb110d513f13b396eb99279affbaf5de975fb159356fc7bc3bec7c6cfd8c68c5","last_reissued_at":"2026-07-05T01:15:08.796570Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:15:08.796570Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"CODEX clusters. The Survey, the Catalog, and Cosmology of the X-ray Luminosity Function","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Finoguenov, C. C. Kirkpatrick, E. Rozo, E. Rykoff, F. Kaefer, G. Erfanianfar, J. Comparat, J. Ider Chitham, J. Patrick Henry, J-P. Kneib, J. Weller, K. Kiiveri, L. van Waerbeke, M. Costanzi, N. Clerc, R. Capasso, R. Dupke, S. Damsted, S. Hagstotz, V. Lindholm","submitted_at":"2019-12-06T17:59:22Z","abstract_excerpt":"Large area catalogs of galaxy clusters constructed from ROSAT All Sky Survey provide the base for our knowledge on the population of clusters thanks to the long-term multiwavelength efforts on their follow-up. Advent of large area photometric surveys superseding in depth previous all-sky data allows us to revisit the construction of X-ray cluster catalogs, extending the study to lower cluster masses and to higher redshifts and to provide the modelling of the selection function. We perform a wavelet detection of X-ray sources and make extensive simulations of the detection of clusters in the RA"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.03262","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1912.03262/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"1912.03262","created_at":"2026-07-05T01:15:08.796632+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.03262v2","created_at":"2026-07-05T01:15:08.796632+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.03262","created_at":"2026-07-05T01:15:08.796632+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZMIQ2UJ7COZZ","created_at":"2026-07-05T01:15:08.796632+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZMIQ2UJ7COZZN24Z","created_at":"2026-07-05T01:15:08.796632+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZMIQ2UJ7","created_at":"2026-07-05T01:15:08.796632+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32","json":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32.json","graph_json":"https://pith.science/api/pith-number/ZMIQ2UJ7COZZN24ZE6NP7OXV32/graph.json","events_json":"https://pith.science/api/pith-number/ZMIQ2UJ7COZZN24ZE6NP7OXV32/events.json","paper":"https://pith.science/paper/ZMIQ2UJ7"},"agent_actions":{"view_html":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32","download_json":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32.json","view_paper":"https://pith.science/paper/ZMIQ2UJ7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.03262&json=true","fetch_graph":"https://pith.science/api/pith-number/ZMIQ2UJ7COZZN24ZE6NP7OXV32/graph.json","fetch_events":"https://pith.science/api/pith-number/ZMIQ2UJ7COZZN24ZE6NP7OXV32/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32/action/storage_attestation","attest_author":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32/action/author_attestation","sign_citation":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32/action/citation_signature","submit_replication":"https://pith.science/pith/ZMIQ2UJ7COZZN24ZE6NP7OXV32/action/replication_record"}},"created_at":"2026-07-05T01:15:08.796632+00:00","updated_at":"2026-07-05T01:15:08.796632+00:00"}